For consistency, these orbit solutions are all products
of our orbit-fitting code applied to the available astrometry
for each binary system (click the object links to see the
astrometry). This occasionally results in somewhat different
solutions from what has appeared in the literature.

Pluto and Haumea were excluded from this
list because those two much more dynamically complex systems
are already being extensively studied by other groups (see,
for example
here and
here).

Additional binaries are also excluded here, if the
identities of the objects have not yet been made public.